1.7k citations · 4.3k across the 36 of their papers we have counts for
36 papers
The VIMOS VLT Deep Survey: Testing the gravitational instability paradigm at z ~ 1
C. Marinoni, L. Guzzo, A. Cappi +5
We have reconstructed the three-dimensional density fluctuation maps to z ~ 1.5 using the distribution of galaxies observed in the VVDS-Deep survey. We use this overdensity field t…
The VVDS type-1 AGN sample: The faint end of the luminosity function
A. Bongiorno, G. Zamorani, I. Gavignaud +51
In a previous paper (Gavignaud et al. 2006), we presented the type-1 Active Galactic Nuclei (AGN) sample obtained from the first epoch data of the VIMOS-VLT Deep Survey (VVDS). The…
Witnessing the build-up of the colour-density relation
O. Cucciati, A. Iovino, C. Marinoni +50
We investigate the redshift and luminosity evolution of the galaxy colour-density relation using the data from the First Epoch VIMOS-VLT Deep Survey (VVDS) on scales of R=5 h^(-1)M…
The cosmic star formation rate evolution from z=5 to z=0 from the VIMOS VLT Deep Survey
L. Tresse, O. Ilbert, E. Zucca +45
We present the evolution of the comoving SFR density in the redshift range 0 < z < 5 using the first epoch data release of the VVDS, that is 11564 spectra selected at I_AB=24 over…
The VIMOS VLT Deep Survey: the faint type-1 AGN sample
I. Gavignaud, A. Bongiorno, S. Paltani +50
We present the type-1 active galactic nuclei (AGN) sample extracted from the VIMOS VLT Deep Survey first observations of 21000 spectra in 1.75 square degree. This sample, which is…
Galaxy luminosity function per morphological type up to z=1.2
O. Ilbert, S. Lauger, L. Tresse +47
We have computed the evolution of the rest-frame B-band luminosity function (LF) for bulge and disk-dominated galaxies since z=1.2. We use a sample of 605 spectroscopic redshifts w…